Results 31 to 40 of about 261,296 (275)

REVERBERATION MEASUREMENTS OF THE INNER RADIUS OF THE DUST TORUS IN 17 SEYFERT GALAXIES [PDF]

open access: yes, 2014
We present the results of a dust reverberation survey for 17 nearby Seyfert 1 galaxies, which provides the largest homogeneous data collection for the radius of the innermost dust torus. A delayed response of the K-band light curve after the V-band light
S. Koshida   +10 more
semanticscholar   +1 more source

Sub-parsec radio cores in nearby Seyfert galaxies [PDF]

open access: yes, 2013
We present a census of sub-pc scale properties of the VLBI cores in a complete sample of local Seyfert galaxies. Seventeen out of 23 sources with a VLA detection are detected also with VLBI at 1.7 GHz and/or 5 GHz, with an average monochromatic radio ...
F. Panessa, M. Giroletti
semanticscholar   +1 more source

The Multitude of Unresolved Continuum Sources at 1.6 microns in Hubble Space Telescope images of Seyfert Galaxies [PDF]

open access: yes, 1999
We examine 112 Seyfert galaxies observed by the Hubble Space Telescope (HST) at 1.6 microns. We find that ~50% of the Seyfert 2.0 galaxies which are part of the Revised Shapeley-Ames (RSA) Catalog or the CfA redshift sample contain unresolved continuum ...
A. Alonso‐Herrero   +18 more
core   +5 more sources

NUCLEAR STAR FORMATION ACTIVITY AND BLACK HOLE ACCRETION IN NEARBY SEYFERT GALAXIES [PDF]

open access: yes, 2013
Recent theoretical and observational works indicate the presence of a correlation between the star-formation rate (SFR) and active galactic nucleus (AGN) luminosity (and, therefore, the black hole accretion rate, ) of Seyfert galaxies.
P. Esquej   +18 more
semanticscholar   +1 more source

X-RAY VARIABILITY STUDY OF POLAR SCATTERED SEYFERT1 GALAXIES

open access: yesActa Polytechnica, 2014
We study 12 Seyfert 1 galaxies with a high level of optical polarization. Optical light emerging from the innermost regions is predominantly scattered in a polar region above the central engine directly in our line of sight.
Tobias Beuchert   +6 more
doaj   +1 more source

Spitzer/IRS Observations of Seyfert 1.8s and 1.9s: A Comparison with Seyfert 1s and Seyfert 2s [PDF]

open access: yes, 2007
We present Spitzer Space Telescope mid-infrared spectra of 12 Seyfert 1.8 and 1.9 galaxies over the 5-38 um region. We compare the spectral characteristics of this sample to those of 58 Seyfert 1 and Seyfert 2 galaxies from the Spitzer archives.
Antonucci R.   +11 more
core   +3 more sources

Optical Properties of Two Complementary Samples of Intermediate Seyfert Galaxies

open access: yesPhysics, 2023
We present first results of the analysis of optical spectra of two complementary samples of Seyfert galaxies (Seyferts). The first sample was extracted from a selection of the 4th Fermi Gamma-ray Large Area Telescope (4FGL) catalog and consists of 11 γ ...
Benedetta Dalla Barba   +5 more
doaj   +1 more source

Unification of X-ray winds in Seyfert galaxies: from ultra-fast outflows to warm absorbers [PDF]

open access: yes, 2012
The existence of ionized X-ray absorbing layers of gas along the line of sight to the nuclei of Seyfert galaxies is a well established observational fact. This material is systematically outflowing and shows a large range in parameters.
F. Tombesi   +12 more
semanticscholar   +1 more source

Radio jets and gamma-ray emission in radio-silent narrow-line Seyfert 1 galaxies [PDF]

open access: yesAstronomy & Astrophysics, 2018
We have detected six narrow-line Seyfert 1 (NLS1) galaxies at 37 GHz that were previously classified as radio silent and two that were classified as radio quiet.
A. Lähteenmäki   +6 more
semanticscholar   +1 more source

Relativistic jets in narrow-line Seyfert 1 galaxies. New discoveries and open questions

open access: yesEPJ Web of Conferences, 2013
Before the launch of the Fermi satellite only two classes of AGNs were known to produce relativistic jets and thus emit up to the γ-ray energy range: blazars and radio galaxies, both hosted in giant elliptical galaxies.
D’Ammando F.   +4 more
doaj   +1 more source

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